- Timestamp:
- Jul 11, 2016, 9:35:35 AM (8 years ago)
- File:
-
- 1 edited
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trunk/DOC/chantiers/commit_importants.log
r1564 r1572 1789 1789 it paves the path for a similar (and, now, easy) counterpart for mesoscale 1790 1790 models 1791 1792 ********************** 1793 **** commit_v1572 **** 1794 ********************** 1795 Ehouarn: Further adaptations to keep up with changes in LMDZ5 concerning 1796 physics/dynamics separation (up to rev r2500 of LMDZ5) 1797 1798 * arch: 1799 - remove ifort debug option '-check all', replace it with 1800 '-check bounds,format,output_conversion,pointers,uninit' (i.e. 1801 get it to stop complaining about copying into temporary arrays) 1802 1803 * dyn3d_common: 1804 - comconst_mod.F90 : add ngroup 1805 1806 * dyn3d: 1807 - gcm.F90 : minor bug fix (arguments to a call_abort()) 1808 - leapfrog.F90 : recompute geopotential for bilan_dyn outputs 1809 - conf_gcm.F90 : read "ngroup" from run.def 1810 - groupe.F , groupeun.F : ngroup no longer a local parameter 1811 1812 * dyn3d_par: 1813 - conf_gcm.F90 : read "ngroup" from run.def 1814 - groupe_p.F , groupeun_p.F : ngroup no longer a local parameter 1815 1816 * misc: 1817 - regr1_step_av_m.F90 : removed (not used) 1818 1819 * phy_common: 1820 - mod_phys_lmdz_mpi_transfert.F90 , mod_phys_lmdz_mpi_data.F90 : change 1821 is_north_pole and is_south_pole to is_north_pole_dyn and is_south_pole_dyn 1822 - mod_phys_lmdz_omp_data.F90 : introduce is_nort_pole_phy and is_south_pole_phy 1823 1824 * dynphy_lonlat: 1825 - mod_interface_dyn_phys.F90 : use is_north_pole_dyn and is_south_pole_dyn 1826 - calfis_p.F : use is_north_pole_dyn and is_south_pole_dyn 1827 1828 * phyvenus: 1829 - physiq_mod , write_hist*.h : use is_north_pole_phy and is_south_pole_phy 1830 to correctly compute mesh area at poles to send to hist*nc files. 1831 1832 * phytitan: 1833 - physiq_mod , write_hist*.h : use is_north_pole_phy and is_south_pole_phy 1834 to correctly compute mesh area at poles to send to hist*nc files.
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